| |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aries |
| Right ascension | 02h42m 21.93980s[1] |
| Declination | +20° 00′ 41.2612″[1] |
| Apparent magnitude (V) | 5.74[2] (6.38/8.38/6.72/12.2)[3] |
| Characteristics | |
| Spectral type | A0 Vp + F2 V + A1 V[3] |
| U−B color index | –0.03[4] |
| B−V color index | –0.02[4] |
| Astrometry | |
| Radial velocity (Rv) | –6.0[5] km/s |
| Proper motion (μ) | RA: +27.68[1] mas/yr Dec.: –47.64[1] mas/yr |
| Parallax (π) | 9.64 ± 0.88 mas[1] |
| Distance | 340 ± 30 ly (104 ± 9 pc) |
| Absolute magnitude (MV) | +0.41[6] |
| Orbit[7] | |
| Period (P) | 8.845 ± 0.046 yr |
| Semi-major axis (a) | 0.0563 ± 0.0008″ |
| Eccentricity (e) | 0.337 ± 0.023 |
| Inclination (i) | 71.2 ± 1.1° |
| Longitude of the node (Ω) | 101.0 ± 1.0° |
| Periastron epoch (T) | B 1981.099 ± 0.063 |
| Argument of periastron (ω) (secondary) | 92.3 ± 1.7° |
| Details | |
| Mass | 3.4 ± 1.7 (Aa) / 2.1 ± 1.7 (Ab)[7] M☉ |
| Luminosity | 71.7[6] L☉ |
| Rotational velocity (v sin i) | 175[8] km/s |
| Other designations | |
μ Ari, 34 Arietis, BD+19 403, HD 16811, HIP 12640, HR 793, SAO 93062.[9] | |
| Database references | |
| SIMBAD | data |
Mu Arietis, Latinized from μ Arietis, is the Bayer designation for a star system in the northern constellationofAries. It is approximately 340 light-years (100 parsecs) distant from Earth, give or take a 30 light-year margin of error, and has a combined apparent visual magnitude of 5.74.[2] According to the Bortle Dark-Sky Scale, this means it is faintly visible to the naked eye from dark suburban skies.
At the heart of this system is a close orbiting pair consisting of a magnitude 6.38 A-type main sequence star with a stellar classification of A0 Vp and a magnitude 8.38 F-type main sequence companion with a classification of F2 V. These two components have an angular separation of 0.04 arcseconds. A third component, consisting of a magnitude 6.72 star with a classification of A1 V, is orbiting the inner pair with a period of 8.845 years and an eccentricity of 0.34. A smaller fourth component, at an angular separation of 19.1 arcseconds, has a magnitude of 12.2.[3]
{{cite web}}: CS1 maint: postscript (link)
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